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20242026
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astro-ph.SR2026

Energy Evolution from the Chromosphere to the Heliosphere in the 2021 October 28 Solar Eruption

Katharine K. Reeves, Daniel B. Seaton, Cynthia Cattell +20

We perform a detailed study of the energetics for a well-observed solar eruption and flare that occurred on 28 October 2021. This event included a GOES class X1.0 flare, a global E…

astro-ph.SR2025

A sudden fine-scale bright kernel captured by Hi-C Flare in 11 MK emission during an M1.6-class solar flare's post-maximum phase

Sanjiv K. Tiwari, Navdeep K. Panesar, Ronald L. Moore +17

On April 17, 2024, the third successful Hi-C sounding rocket flight, Hi-C Flare, recorded coronal images in Fe XXI 129 A emission from 11 MK plasma during the post-maximum phase of…

astro-ph.SR2025

Disentangling Thermal and Abundance Characteristics in a Solar Flare Using SDO/AIA, Hinode/XRT, and MinXSS-1 Observations

Xiaoyan Xie, Anna Chen, Crisel Suarez +5

We investigate the thermal properties of a solar flare by the observations of soft X-ray Telescope (XRT) on board Hinode and the Atmospheric Image Assembly on board the Solar Dynam…

astro-ph.SR2025

Supra-arcade downflows in an extensive fan associated with a giant quiescent solar filament eruption

Xiaoyan Xie, Katharine Reeves, Chengcai Shen +6

We investigate the aftermath of a giant quiescent solar filament eruption on December 24, 2023. One feature of the eruption is an extensive fan above the filament channel that is a…

astro-ph.SR2024

Determining the nanoflare heating frequency of an X-ray Bright Point observed by MaGIXS

Biswajit Mondal, P. S. Athiray, Amy R. Winebarger +18

Nanoflares are thought to be one of the prime candidates that can heat the solar corona to its multi-million kelvin temperature. Individual nanoflares are difficult to detect with…